Viewing archive of Friday, 25 October 2002

Solar activity report

Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Report of Solar-Geophysical Activity 2002 Oct 25 2200 UTC
Prepared by the NOAA © SWPC and processed by SpaceWeatherLive.com

Joint USAF/NOAA Report of Solar and Geophysical Activity

SDF Number 298 Issued at 2200Z on 25 Oct 2002

IA. Analysis of Solar Active Regions and Activity from 24-2100Z to 25-2100Z

Solar activity increased to moderate levels. Region 162 (N26W18) produced a long duration M1.5/1f event at 25/1747 UTC along with multiple C-class flares today. The M1.5/1f flare produced an associated Type II (estimated shock velocity of 389 km/s) and a Type IV radio sweep. SOHO/LASCO imagery was insufficient at the time of this writing to determine whether an earth-directed CME accompanied this flare. This region retains a small delta magnetic structure that has underwent slight decay since yesterday. A disappearing solar filament (approximately 67 heliographic degrees) was seen to dissipate around 25/0600 UTC in the southeast quadrant of the disk. Two separate H-class spot groups were newly assigned today, Regions 170 (S12E65) and 171 (N10E76).
IB. Solar Activity Forecast
Solar activity is expected to be at moderate levels due to the magnetic complexity of Region 162.
IIA. Geophysical Activity Summary 24-2100Z to 25-2100Z
The geomagnetic field was at unsettled to major storm levels. The large coronal hole in the western solar hemisphere continues to elevate the high speed solar wind (approximate average speed of 700 km/s). The greater than 2 MeV electron flux at geosynchronous orbit reached moderate levels today.
IIB. Geophysical Activity Forecast
The geomagnetic field is expected to be at quiet to minor storm levels. The coronal hole high speed stream effects should persist through day one and into day two of the forecast period, returning to predominantly quiet to unsettled conditions by day three.
III. Event Probabilities 26 Oct to 28 Oct
Class M50%50%50%
Class X05%05%05%
Proton05%05%05%
PCAFyellow
IV. Penticton 10.7 cm Flux
  Observed       25 Oct 173
  Predicted   26 Oct-28 Oct  170/170/170
  90 Day Mean        25 Oct 179
V. Geomagnetic A Indices
  Observed Afr/Ap 24 Oct  022/047
  Estimated     Afr/Ap 25 Oct  035/040
  Predicted    Afr/Ap 26 Oct-28 Oct  025/025-015/015-010/012
VI. Geomagnetic Activity Probabilities 26 Oct to 28 Oct
A. Middle Latitudes
Active40%25%20%
Minor storm10%10%05%
Major-severe storm05%05%01%
B. High Latitudes
Active50%30%25%
Minor storm15%15%05%
Major-severe storm10%05%01%

All times in UTC

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